The ballistic sorting effect has been proposed to be a driver behind the observed size sorting on the rubble pile asteroid Itokawa. This effect depends on the inelasticity of slow collisions with granular materials. The inelasticity of a collision with a granular material, in turn, depends on grain size. Here we argue that determining the inelasticity of such collisions in an asteroid-like environment is a nontrivial task. We show non-monotonic dependency of the coefficient of restitution (COR) on target particle size using experiments in microgravity. Employing numerical simulations, we explain these results with the growing influence of adhesion for smaller-sized particles. We conclude that there exists an optimum impactor to target particle size ratio for ballistic sorting.
机构:
Chinese Acad Sci, Purple Mt Observ, CAS Key Lab Planetary Sci, Nanjing 210023, Peoples R China
CAS Ctr Excellence Comparat Planetol, Hefei 230026, Peoples R ChinaChinese Acad Sci, Purple Mt Observ, CAS Key Lab Planetary Sci, Nanjing 210023, Peoples R China
Hu, Shoucun
Richardson, Derek C.
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Univ Maryland, Dept Astron, College Pk, MD 20742 USAChinese Acad Sci, Purple Mt Observ, CAS Key Lab Planetary Sci, Nanjing 210023, Peoples R China
Richardson, Derek C.
Zhang, Yun
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Univ Cote Azur, Observ Cote Azur, Lab Lagrange, CNRS, F-06304 Nice, FranceChinese Acad Sci, Purple Mt Observ, CAS Key Lab Planetary Sci, Nanjing 210023, Peoples R China
Zhang, Yun
Ji, Jianghui
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Chinese Acad Sci, Purple Mt Observ, CAS Key Lab Planetary Sci, Nanjing 210023, Peoples R China
CAS Ctr Excellence Comparat Planetol, Hefei 230026, Peoples R ChinaChinese Acad Sci, Purple Mt Observ, CAS Key Lab Planetary Sci, Nanjing 210023, Peoples R China